Here we contribute to the study of the HAeBe regime by providing a homogeneous characterization of the stellar and circumstellar properties of most of these confirmed sources, based on their complete SEDs from multiwavelength photometry. For all stars we make use of the recent Gaia Early Data Release 3 [1]}, [2]} parallaxes and photometry [3]}, [4]}. Sect.  describes how the stellar and disk parameters were obtained using the same procedure for all stars, as well as the online archive in which these data are publicly available. Sect.  serves to exemplify the potential use of our dataset for the study of the HAeBe regime. It includes some general statistics that is mainly focused on the analysis of the different circumstellar properties of HAes and HBes as inferred from their SEDs. Finally, Sect.  includes a brief summary and conclusions.
